Speaker
Álvaro Cendal
(Universidad Complutense de Madrid)
Description
Dark matter may not be completely stable, and its decay could lead to new signatures in the form of gravitational waves. In this talk I will present model-independent predictions for the stochastic gravitational wave background produced by dark matter decaying into gravitons. Using this framework, I forecast the sensitivity of current and upcoming gravitational wave detectors to these signals.
Author
Álvaro Cendal
(Universidad Complutense de Madrid)